Published 1983
| Version v1
Book
IUE spectra of RS CVn stars
Creators
- 1. Armagh Observatory, Northern Ireland (UK)
- 2. Colorado Univ., Boulder (USA)
- 3. Catania Univ. (Italy). Osservatorio Astrofisico
Description
Evidence is presented that in RS CVn stars the UV chromospheric and transition region line fluxes vary such that maximum line flux corresponds to optical minimum or maximum spot visibility. This is consistent with a solar-type dark spot model. (Auth.)
Additional details
Publishing Information
- Publisher
- D. Reidel.
- Imprint Place
- Dordrecht (Netherlands)
- ISBN
- 90-277-1601-3
- Imprint Title
- Activity in red-dwarf stars
- Imprint Pagination
- 669 p.
- Journal Volume
- 102
- Series
- Astrophysics and space science library.
- Journal Page Range
- p. 444-445.
Conference
- Title
- 71. Colloquium of the International Astronomical Union.
- Dates
- 10-13 Aug 1982.
- Place
- Catania (Italy).
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 15023495
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference, Numerical Data
- Descriptors DEI
- BINARY STARS; EMISSION SPECTRA; EXPERIMENTAL DATA; PHOTOMETRY; SPECTROSCOPY; STELLAR CORONAE; STELLAR FLARES; VISIBLE RADIATION
- Descriptors DEC
- ATMOSPHERES; DATA; ELECTROMAGNETIC RADIATION; INFORMATION; NUMERICAL DATA; RADIATIONS; SPECTRA; STARS; STELLAR ATMOSPHERES
Optional Information
- Notes
- 4 figs. Imprint:Includes subject index.